most citedMagnetocentrifugal Winds in 3D: Nonaxisymmetric Steady State

26 citations · 26 across the 1 of their papers we have counts for

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5 papers

astro-ph200626 cited

Magnetocentrifugal Winds in 3D: Nonaxisymmetric Steady State

Jeffrey M. Anderson, Zhi-Yun Li, Ruben Krasnopolsky +1

Outflows can be loaded and accelerated to high speeds along rapidly rotating, open magnetic field lines by centrifugal forces. Whether such magnetocentrifugally driven winds are st…

astro-ph2005

Nonlinear Criterion for the Stability of Molecular Clouds

Ruben Krasnopolsky, Charles F. Gammie

Dynamically significant magnetic fields are routinely observed in molecular clouds, with mass-to-flux ratio lambda = (2 pi sqrt{G}) (Sigma/B) ~ 1 (here Sigma is the total column de…

astro-ph2004

The Structure of Magnetocentrifugal Winds I. Steady Mass Loading

Jeffrey M. Anderson, Zhi-Yun Li, Ruben Krasnopolsky +1

We present the results of a series of time-dependent numerical simulations of cold, magnetocentrifugally launched winds from accretion disks. Our simulations span four and half dec…

astro-ph2003

Magneto-Centrifugal Launching of Jets from Accretion Disks. II: Inner Disk-Driven Winds

Ruben Krasnopolsky, Zhi-Yun Li, Roger D. Blandford

We follow numerically the time evolution of axisymmetric outflows driven magneto-centrifugally from the inner portion of accretion disks, from their launching surface to large, obs…

astro-ph2003

Locating the Launching Region of T Tauri Winds: The Case of DG Tau

Jeffrey M. Anderson, Zhi-Yun Li, Ruben Krasnopolsky +1

It is widely believed that T Tauri winds are driven magnetocentrifugally from accretion disks close to the central stars. The exact launching conditions are uncertain. We show that…